HSC 2733

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0.03 UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.06
Cdup
Radius (P>50% members) 76.0 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.06 Very likely duplicate

Overview

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HSC 2733 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a low-mass, near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very close Low extinction Low mass Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 227.975 -44.303 6.843 -20.592 -21.945 5.34
Hunt & Reffert 2024 228.065 -44.529 6.849 -20.667 -21.892 2.664
Cavallo et al. 2024 227.786 -43.966 6.849 – – –
Hunt & Reffert 2023 228.065 -44.529 6.849 -20.667 -21.892 2.664

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfr BSS
Hunt & Reffert 2024 – – – – – 40* – –
Cavallo et al. 2024 0.14 0.66 – 19 0.100 – – –
Hunt & Reffert 2023 0.14 0.14 0.40 10 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 320 94.3 228.12 -44.14 6.81 -20.5 -21.89 4.7 0.55

💡 Note: The % column shows the percentage of members that HSC 2733 shares with each listed object.

Visualization

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